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- W4290691786 abstract "Context. Millisecond pulsars (MSPs) represent nearly half of the more than 160 currently known γ-ray pulsars detected by the Large Area Telescope on the Fermi satellite, and a third of all known MSPs are seen in γ rays. The least energetic γ-ray MSPs enable us to probe the so-called deathline for high-energy emission, i.e., the spin-down luminosity limit under which pulsars (PSRs) cease to produce detectable high-energy radiation. Characterizing the MSP luminosity distribution helps to determine their contribution to the Galactic diffuse γ-ray emission." @default.
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- W4290691786 date "2016-02-26" @default.
- W4290691786 modified "2023-10-02" @default.
- W4290691786 title "The gamma-ray millisecond pulsar deathline, revisited" @default.
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- W4290691786 doi "https://doi.org/10.1051/0004-6361/201527847" @default.
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